Perseus and Camelopardalis 4h 30m 5′ 4h 00m 3h 30m 3h 00m Star magnitudes King 4 King 6 d +55° a King 5 o King 7 h + 5′ +60° CAS CAMELOPARDALIS 2 3 4 5 6 7 2h 30m _ PERSEUS e +50° f b pp KING 8 The first of three targets in Auriga, King 8 is a very easy open cluster with no concentration toward its center. Made up of a moderate population of mostly bright stars, the range of magnitudes in the cluster is small, as per its Trumpler classification. Mv = 11.2 | S = 4′ | No. = 198 | Tr = II2m | Mag. = 77× p KING 17 The star field can be found easily, though this open cluster is very small and very faint. Mv* = 14 | S = 5′ | No. = 25 | Tr = II2m | Mag. = 337× +45° q KING 22 A very open cluster that is easily missed, King 22 (also known as Berkeley 18) is around 1° southeast of Capella. I only noted bright members, but maybe poor transparency made it difficult to separate the fainter stars. Mv* = 16 | S = 12′ | No. = 300 | Tr = III1r | Mag. = 66× and 256× 5′ sk yandtele scope.com * N OV E M B E R 2 019 65http://www.skyandtelescope.com